Coverage for python/lsst/meas/algorithms/measureApCorr.py: 16%
164 statements
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1#
2# LSST Data Management System
3#
4# Copyright 2008-2017 AURA/LSST.
5#
6# This product includes software developed by the
7# LSST Project (http://www.lsst.org/).
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14# This program is distributed in the hope that it will be useful,
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17# GNU General Public License for more details.
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21# see <https://www.lsstcorp.org/LegalNotices/>.
22#
24__all__ = ("MeasureApCorrConfig", "MeasureApCorrTask", "MeasureApCorrError")
26import numpy as np
27from scipy.stats import median_abs_deviation
29import lsst.pex.config
30from lsst.afw.image import ApCorrMap
31from lsst.afw.math import ChebyshevBoundedField, ChebyshevBoundedFieldConfig
32from lsst.pipe.base import Task, Struct, AlgorithmError
33from lsst.meas.base.apCorrRegistry import getApCorrNameSet
35from .sourceSelector import sourceSelectorRegistry
38class MeasureApCorrError(AlgorithmError):
39 """Raised if Aperture Correction fails in a non-recoverable way.
41 Parameters
42 ----------
43 name : `str`
44 Name of the kind of aperture correction that failed; typically an
45 instFlux catalog field.
46 nSources : `int`
47 Number of sources available to the fitter at the point of failure.
48 ndof : `int`
49 Number of degrees of freedom required at the point of failure.
50 iteration : `int`, optional
51 Which fit iteration the failure occurred in.
52 """
53 def __init__(self, *, name, nSources, ndof, iteration=None):
54 msg = f"Unable to measure aperture correction for '{name}'"
55 if iteration is not None:
56 msg += f" after {iteration} steps:"
57 else:
58 msg += ":"
59 msg += f" only {nSources} sources, but require at least {ndof}."
60 super().__init__(msg)
61 self.name = name
62 self.nSources = nSources
63 self.ndof = ndof
64 self.iteration = iteration
66 @property
67 def metadata(self):
68 metadata = {"name": self.name,
69 "nSources": self.nSources,
70 "ndof": self.ndof,
71 }
72 # NOTE: have to do this because task metadata doesn't allow None.
73 if self.iteration is not None:
74 metadata["iteration"] = self.iteration
75 return metadata
78class _FluxNames:
79 """A collection of flux-related names for a given flux measurement algorithm.
81 Parameters
82 ----------
83 name : `str`
84 Name of flux measurement algorithm, e.g. ``base_PsfFlux``.
85 schema : `lsst.afw.table.Schema`
86 Catalog schema containing the flux field. The ``{name}_instFlux``,
87 ``{name}_instFluxErr``, ``{name}_flag`` fields are checked for
88 existence, and the ``apcorr_{name}_used`` field is added.
90 Raises
91 ------
92 KeyError if any of instFlux, instFluxErr, or flag fields is missing.
93 """
94 def __init__(self, name, schema):
95 self.fluxName = name + "_instFlux"
96 if self.fluxName not in schema:
97 raise KeyError("Could not find " + self.fluxName)
98 self.errName = name + "_instFluxErr"
99 if self.errName not in schema:
100 raise KeyError("Could not find " + self.errName)
101 self.flagName = name + "_flag"
102 if self.flagName not in schema:
103 raise KeyError("Cound not find " + self.flagName)
104 self.usedName = "apcorr_" + name + "_used"
105 schema.addField(self.usedName, type="Flag",
106 doc="Set if source was used in measuring aperture correction.")
109class MeasureApCorrConfig(lsst.pex.config.Config):
110 """Configuration for MeasureApCorrTask.
111 """
112 refFluxName = lsst.pex.config.Field(
113 doc="Field name prefix for the flux other measurements should be aperture corrected to match",
114 dtype=str,
115 default="slot_CalibFlux",
116 )
117 sourceSelector = sourceSelectorRegistry.makeField(
118 doc="Selector that sets the stars that aperture corrections will be measured from.",
119 default="science",
120 )
121 minDegreesOfFreedom = lsst.pex.config.RangeField(
122 doc="Minimum number of degrees of freedom (# of valid data points - # of parameters);"
123 " if this is exceeded, the order of the fit is decreased (in both dimensions), and"
124 " if we can't decrease it enough, we'll raise ValueError.",
125 dtype=int,
126 default=1,
127 min=1,
128 )
129 fitConfig = lsst.pex.config.ConfigField(
130 doc="Configuration used in fitting the aperture correction fields.",
131 dtype=ChebyshevBoundedFieldConfig,
132 )
133 numIter = lsst.pex.config.Field(
134 doc="Number of iterations for robust MAD sigma clipping.",
135 dtype=int,
136 default=4,
137 )
138 numSigmaClip = lsst.pex.config.Field(
139 doc="Number of robust MAD sigma to do clipping.",
140 dtype=float,
141 default=4.0,
142 )
143 allowFailure = lsst.pex.config.ListField(
144 doc="Allow these measurement algorithms to fail without an exception.",
145 dtype=str,
146 default=[],
147 )
149 def setDefaults(self):
150 selector = self.sourceSelector["science"]
152 selector.doFlags = True
153 selector.doUnresolved = True
154 selector.doSignalToNoise = True
155 selector.doIsolated = False
156 selector.flags.good = []
157 selector.flags.bad = [
158 "base_PixelFlags_flag_edge",
159 "base_PixelFlags_flag_interpolatedCenter",
160 "base_PixelFlags_flag_saturatedCenter",
161 "base_PixelFlags_flag_crCenter",
162 "base_PixelFlags_flag_bad",
163 "base_PixelFlags_flag_interpolated",
164 "base_PixelFlags_flag_saturated",
165 ]
166 selector.signalToNoise.minimum = 200.0
167 selector.signalToNoise.maximum = None
168 selector.signalToNoise.fluxField = "base_PsfFlux_instFlux"
169 selector.signalToNoise.errField = "base_PsfFlux_instFluxErr"
171 def validate(self):
172 lsst.pex.config.Config.validate(self)
173 if self.sourceSelector.target.usesMatches:
174 raise lsst.pex.config.FieldValidationError(
175 MeasureApCorrConfig.sourceSelector,
176 self,
177 "Star selectors that require matches are not permitted.")
180class MeasureApCorrTask(Task):
181 """Task to measure aperture correction.
182 """
183 ConfigClass = MeasureApCorrConfig
184 _DefaultName = "measureApCorr"
186 def __init__(self, schema, **kwargs):
187 """Construct a MeasureApCorrTask
189 For every name in lsst.meas.base.getApCorrNameSet():
190 - If the corresponding flux fields exist in the schema:
191 - Add a new field apcorr_{name}_used
192 - Add an entry to the self.toCorrect dict
193 - Otherwise silently skip the name
194 """
195 Task.__init__(self, **kwargs)
196 self.refFluxNames = _FluxNames(self.config.refFluxName, schema)
197 self.toCorrect = {} # dict of flux field name prefix: FluxKeys instance
198 for name in sorted(getApCorrNameSet()):
199 try:
200 self.toCorrect[name] = _FluxNames(name, schema)
201 except KeyError:
202 # if a field in the registry is missing, just ignore it.
203 pass
204 self.makeSubtask("sourceSelector")
206 def run(self, exposure, catalog):
207 """Measure aperture correction
209 Parameters
210 ----------
211 exposure : `lsst.afw.image.Exposure`
212 Exposure aperture corrections are being measured on. The
213 bounding box is retrieved from it, and it is passed to the
214 sourceSelector. The output aperture correction map is *not*
215 added to the exposure; this is left to the caller.
216 catalog : `lsst.afw.table.SourceCatalog`
217 SourceCatalog containing measurements to be used to
218 compute aperture corrections.
220 Returns
221 -------
222 Struct : `lsst.pipe.base.Struct`
223 Contains the following:
225 ``apCorrMap``
226 aperture correction map (`lsst.afw.image.ApCorrMap`)
227 that contains two entries for each flux field:
228 - flux field (e.g. base_PsfFlux_instFlux): 2d model
229 - flux sigma field (e.g. base_PsfFlux_instFluxErr): 2d model of error
230 """
231 bbox = exposure.getBBox()
232 import lsstDebug
233 display = lsstDebug.Info(__name__).display
234 doPause = lsstDebug.Info(__name__).doPause
236 self.log.info("Measuring aperture corrections for %d flux fields", len(self.toCorrect))
238 # First, create a subset of the catalog that contains only selected stars
239 # with non-flagged reference fluxes.
240 selected = self.sourceSelector.run(catalog, exposure=exposure)
242 use = (
243 ~selected.sourceCat[self.refFluxNames.flagName]
244 & (np.isfinite(selected.sourceCat[self.refFluxNames.fluxName]))
245 )
246 goodRefCat = selected.sourceCat[use].copy()
248 apCorrMap = ApCorrMap()
250 # Outer loop over the fields we want to correct
251 for name, fluxNames in self.toCorrect.items():
252 # Create a more restricted subset with only the objects where the to-be-correct flux
253 # is not flagged.
254 fluxes = goodRefCat[fluxNames.fluxName]
255 with np.errstate(invalid="ignore"): # suppress NaN warnings.
256 isGood = (
257 (~goodRefCat[fluxNames.flagName])
258 & (np.isfinite(fluxes))
259 & (fluxes > 0.0)
260 )
262 # The 1 is the minimum number of ctrl.computeSize() when the order
263 # drops to 0 in both x and y.
264 if (isGood.sum() - 1) < self.config.minDegreesOfFreedom:
265 if name in self.config.allowFailure:
266 self.log.warning("Unable to measure aperture correction for '%s': "
267 "only %d sources, but require at least %d.",
268 name, isGood.sum(), self.config.minDegreesOfFreedom + 1)
269 continue
270 else:
271 raise MeasureApCorrError(name=name, nSources=isGood.sum(),
272 ndof=self.config.minDegreesOfFreedom + 1)
274 goodCat = goodRefCat[isGood].copy()
276 x = goodCat['slot_Centroid_x']
277 y = goodCat['slot_Centroid_y']
278 z = goodCat[self.refFluxNames.fluxName]/goodCat[fluxNames.fluxName]
279 ids = goodCat['id']
281 # We start with an initial fit that is the median offset; this
282 # works well in practice.
283 fitValues = np.median(z)
285 ctrl = self.config.fitConfig.makeControl()
287 allBad = False
288 for iteration in range(self.config.numIter):
289 resid = z - fitValues
290 # We add a small (epsilon) amount of floating-point slop because
291 # the median_abs_deviation may give a value that is just larger than 0
292 # even if given a completely flat residual field (as in tests).
293 apCorrErr = median_abs_deviation(resid, scale="normal") + 1e-7
294 keep = np.abs(resid) <= self.config.numSigmaClip * apCorrErr
296 self.log.debug("Removing %d sources as outliers.", len(resid) - keep.sum())
298 x = x[keep]
299 y = y[keep]
300 z = z[keep]
301 ids = ids[keep]
303 while (len(x) - ctrl.computeSize()) < self.config.minDegreesOfFreedom:
304 if ctrl.orderX > 0:
305 ctrl.orderX -= 1
306 else:
307 allBad = True
308 break
309 if ctrl.orderY > 0:
310 ctrl.orderY -= 1
311 else:
312 allBad = True
313 break
315 if allBad:
316 if name in self.config.allowFailure:
317 self.log.warning("Unable to measure aperture correction for '%s': "
318 "only %d sources remain, but require at least %d." %
319 (name, keep.sum(), self.config.minDegreesOfFreedom + 1))
320 break
321 else:
322 raise MeasureApCorrError(name=name, nSources=keep.sum(),
323 ndof=self.config.minDegreesOfFreedom + 1,
324 iteration=iteration+1)
326 apCorrField = ChebyshevBoundedField.fit(bbox, x, y, z, ctrl)
327 fitValues = apCorrField.evaluate(x, y)
329 if allBad:
330 continue
332 self.log.info(
333 "Aperture correction for %s from %d stars: MAD %f, RMS %f",
334 name,
335 len(x),
336 median_abs_deviation(fitValues - z, scale="normal"),
337 np.mean((fitValues - z)**2.)**0.5,
338 )
340 if display:
341 plotApCorr(bbox, x, y, z, apCorrField, "%s, final" % (name,), doPause)
343 # Record which sources were used.
344 used = np.zeros(len(catalog), dtype=bool)
345 used[np.searchsorted(catalog['id'], ids)] = True
346 catalog[fluxNames.usedName] = used
348 # Save the result in the output map
349 # The error is constant spatially (we could imagine being
350 # more clever, but we're not yet sure if it's worth the effort).
351 # We save the errors as a 0th-order ChebyshevBoundedField
352 apCorrMap[fluxNames.fluxName] = apCorrField
353 apCorrMap[fluxNames.errName] = ChebyshevBoundedField(
354 bbox,
355 np.array([[apCorrErr]]),
356 )
358 return Struct(
359 apCorrMap=apCorrMap,
360 )
363def plotApCorr(bbox, xx, yy, zzMeasure, field, title, doPause):
364 """Plot aperture correction fit residuals
366 There are two subplots: residuals against x and y.
368 Intended for debugging.
370 Parameters
371 ----------
372 bbox : `lsst.geom.Box2I`
373 Bounding box (for bounds)
374 xx, yy : `numpy.ndarray`, (N)
375 x and y coordinates
376 zzMeasure : `float`
377 Measured value of the aperture correction
378 field : `lsst.afw.math.ChebyshevBoundedField`
379 Fit aperture correction field
380 title : 'str'
381 Title for plot
382 doPause : `bool`
383 Pause to inspect the residuals plot? If
384 False, there will be a 4 second delay to
385 allow for inspection of the plot before
386 closing it and moving on.
387 """
388 import matplotlib.pyplot as plt
390 zzFit = field.evaluate(xx, yy)
391 residuals = zzMeasure - zzFit
393 fig, axes = plt.subplots(2, 1)
395 axes[0].scatter(xx, residuals, s=3, marker='o', lw=0, alpha=0.7)
396 axes[1].scatter(yy, residuals, s=3, marker='o', lw=0, alpha=0.7)
397 for ax in axes:
398 ax.set_ylabel("ApCorr Fit Residual")
399 ax.set_ylim(0.9*residuals.min(), 1.1*residuals.max())
400 axes[0].set_xlabel("x")
401 axes[0].set_xlim(bbox.getMinX(), bbox.getMaxX())
402 axes[1].set_xlabel("y")
403 axes[1].set_xlim(bbox.getMinY(), bbox.getMaxY())
404 plt.suptitle(title)
406 if not doPause:
407 try:
408 plt.pause(4)
409 plt.close()
410 except Exception:
411 print("%s: plt.pause() failed. Please close plots when done." % __name__)
412 plt.show()
413 else:
414 print("%s: Please close plots when done." % __name__)
415 plt.show()